A symplectic mapping model as a tool to understand the dynamics of 2/1 resonant asteroid motion

DOI10.1023/A:1008378426081zbMath0960.70013MaRDI QIDQ1976072

John D. Hadjidemetriou

Publication date: 1999

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)

zbMATH Keywords

Poincaré mapsymplectic model2:1 mean motion resonanceSun-Jupiter-astroidthree body-problem

Mathematics Subject Classification ID

Celestial mechanics (70F15) Dynamical systems in classical and celestial mechanics (37N05)

Related Items (5)

The dynamical structure of the MEO region: long-term stability, chaos, and transport ⋮ ON THE BIFURCATION AND CONTINUATION OF PERIODIC ORBITS IN THE THREE BODY PROBLEM ⋮ Dynamic expansion points: an extension to Hadjidemetriou's mapping method ⋮ A symplectic mapping for the synchronous spin-orbit problem ⋮ Formal solution of the asteroid motion near the 2:1 commensurability

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